Add to ORKGThree theoretical problems concerning the large scale structure of disk galaxies in general, and the Milky Way System, in particular, were proposed to study. They are, namely, modes of spiral density waves, evolutionary change of the abundance distribution of the gas in the Milky Way System and the motions of the cloud medium behind the large scale galactic shock
The general association of luminous young stars with spiral arms in galaxies has led to widespread a...
Results from numerical simulations of normal isolated late-type spiral galaxies are presented; speci...
Molecular clouds are imperative to astronomy as the sites of all known star formation. The problem o...
The dynamics of spiral galaxies is a gold-mine of challenging problems for the astrophysicist and th...
How does it happen that billions of stars can cooperate to produce the beautiful spirals that charac...
The generation of transient spiral waves by swing-amplification in self-gravitating disks is now reg...
[[abstract]]The density-wave theory of galactic spirals is developed in a form slightly more general...
[[abstract]]Axisymmetric models of disk galaxies taken together with the density wave theory allow o...
International audienceThis paper is the third in a series of articles devoted to the determination o...
Original paper can be found at http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomi...
The dynamics of stars and gas appear markedly different in flocculent, tidally induced and quasi-sta...
After almost fifty years the origin of spiral arms in disk galaxies remains one of the major unsolve...
We study the large-scale dynamics of the interstellar medium in barred galaxies. The interest in doi...
[[abstract]]We follow the perturbations in the flow of interstellar gas which result from steady for...
Thesis. 1976. M.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Mic...
The general association of luminous young stars with spiral arms in galaxies has led to widespread a...
Results from numerical simulations of normal isolated late-type spiral galaxies are presented; speci...
Molecular clouds are imperative to astronomy as the sites of all known star formation. The problem o...
The dynamics of spiral galaxies is a gold-mine of challenging problems for the astrophysicist and th...
How does it happen that billions of stars can cooperate to produce the beautiful spirals that charac...
The generation of transient spiral waves by swing-amplification in self-gravitating disks is now reg...
[[abstract]]The density-wave theory of galactic spirals is developed in a form slightly more general...
[[abstract]]Axisymmetric models of disk galaxies taken together with the density wave theory allow o...
International audienceThis paper is the third in a series of articles devoted to the determination o...
Original paper can be found at http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomi...
The dynamics of stars and gas appear markedly different in flocculent, tidally induced and quasi-sta...
After almost fifty years the origin of spiral arms in disk galaxies remains one of the major unsolve...
We study the large-scale dynamics of the interstellar medium in barred galaxies. The interest in doi...
[[abstract]]We follow the perturbations in the flow of interstellar gas which result from steady for...
Thesis. 1976. M.S.--Massachusetts Institute of Technology. Dept. of Earth and Planetary Sciences.Mic...
The general association of luminous young stars with spiral arms in galaxies has led to widespread a...
Results from numerical simulations of normal isolated late-type spiral galaxies are presented; speci...
Molecular clouds are imperative to astronomy as the sites of all known star formation. The problem o...